ar X iv : a st ro - p h / 05 02 12 1 v 1 5 F eb 2 00 5 TWO - MIRROR SCHWARZSCHILD APLANATS . BASIC RELATIONS ∗

ar X iv : a st ro - p h / 05 12 61 7 v 1 2 7 D ec 2 00 5 3 D Spectroscopy of Herbig - Haro objects

ar X iv : a st ro - p h / 05 02 23 2 v 1 11 F eb 2 00 5 Supernova neutrino challenges

A principal ‘supernova neutrino challenge’ is the computational difficulty of six-dimensional neutrino radiation hydrodynamics. The variety of resulting approximations has provoked a long history of uncertainty in the core-collapse supernova explosion mechanism, but recent work highlighting low-mode convection and a newlyrecognized instability in spherical accretion shocks may signal (yet anoth...

ar X iv : a st ro - p h / 99 02 06 2 v 1 4 F eb 1 99 9 SOURCES OF RELATIVISTIC JETS IN THE GALAXY

ar X iv : a st ro - p h / 02 08 09 2 v 1 5 A ug 2 00 2 3 - D GRMHD Simulations of Generating Jets

We have performed a first fully 3-D GRMHD simulation with Schwarzschild black hole with a free falling corona. The initial simulation results show that a jet is created as in the previous simulations using the axisymmetric geometry with the mirror symmetry at the equator. However, the time to generate the jet is longer than in the 2-D axisymmetric simulations. We expect that due to the addition...

ar X iv : a st ro - p h / 02 03 41 7 v 1 2 3 M ar 2 00 2 Clustering at high redshift

1 ST European Coordinating Facility, European Southern Observatory, K.-Schwarzschild-Strasse 2, D-85748 Garching bei Muenchen, Germany 2 Osservatorio Astronomico di Trieste, via Tiepolo 11, I-34131 Trieste, Italy 3 European Southern Observatory, K.-Schwarzschild-Strasse 2, D-85748 Garching bei Muenchen, Germany 4 Osservatorio Astronomico di Roma, via dell’Osservatorio 2, Monteporzio, Italy 5 Os...